All Figures

$\begin{figure} \par\includegraphics[height=14cm,width=16.2cm,clip]{odin6_f1.eps} \end{figure}$ Figure 1: The Odin 557 GHz H₂O map. The increments of the velocity and intensity axes are given next to the top right spectrum. The map origin corresponds to J2000 coordinates $\alpha$ = 05 $^{\rm h}$ 35 $^{\rm m}$ 14 $.\!\!^{\rm s}$ 4, $\delta =-05\hbox {$^\circ $ }22\hbox {$^\prime $ }30\hbox {$^{\prime \prime }$ }$ . Lower right insert: one of the two sinusoids subtracted from each scan in the two water map observations in order to compensate for a standing wave phenomenon. Note here the magnified intensity scale.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{odin6_f2.eps} \end{figure}$ Figure 2: H₂O spectra $^\textrm{\scriptsize 2}$ from Fig. 1 along a line of constant declination (2 $^\prime$ south of Orion KL). The sequence goes from west to east in steps of 1 $^\prime$ from bottom to top (the offsets are given at the right hand side).
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{odin6_f3.eps} \end{figure}$ Figure 3: H₂O declination-velocity diagram through Orion KL. The colour coding goes from black ( $\leq$ 1 K), to white ( $\geq$ 7 K). The contours $^\textrm{\scriptsize 2}$ start at 1 K and are incremented with 1.5 K.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{odin6_f4.eps} \end{figure}$ Figure 4: From top to bottom: H₂O (Odin beam 2.1 $^\prime$ ), SiO (Onsala; beam size 0.7 $^\prime$ ), and (Odin) H₂¹⁸O (accompanied by an SO₂ emission line at $\sim$ -60 $\rm km~s^{-1}$ , see text). Note the different vertical scales $^\textrm{\scriptsize 2}$ .
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{odin6_f5.eps} \end{figure}$ Figure 5: H₂¹⁸O towards 2 $^\prime$ south of Orion KL $^\textrm{\scriptsize 2}$ . a) The two separate sky-switched spectra (observed at the dates indicated in the figure) with additional reference positions subtracted. The upper spectrum has been offset upwards with 0.2 K. b) The same observations clipped and RMS averaged after polynomial baseline subtractions (see text for further details).
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{odin6_f6.eps} \end{figure}$ Figure 6: The spectra of Fig. 4 scaled $^\textrm{\scriptsize 2}$ according to the legend. Note that the SiO profile was corrected for the OSO 20 m beam efficiency before scaling.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{odin6_f2.eps} \end{figure}$	Figure 2: H₂O spectra $^\textrm{\scriptsize 2}$ from Fig. 1 along a line of constant declination (2 $^\prime$ south of Orion KL). The sequence goes from west to east in steps of 1 $^\prime$ from bottom to top (the offsets are given at the right hand side).
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$\begin{figure} \par\includegraphics[width=8.8cm,clip]{odin6_f3.eps} \end{figure}$	Figure 3: H₂O declination-velocity diagram through Orion KL. The colour coding goes from black ( $\leq$ 1 K), to white ( $\geq$ 7 K). The contours $^\textrm{\scriptsize 2}$ start at 1 K and are incremented with 1.5 K.
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$\begin{figure} \par\includegraphics[width=8.8cm,clip]{odin6_f4.eps} \end{figure}$	Figure 4: From top to bottom: H₂O (Odin beam 2.1 $^\prime$ ), SiO (Onsala; beam size 0.7 $^\prime$ ), and (Odin) H₂¹⁸O (accompanied by an SO₂ emission line at $\sim$ -60 $\rm km~s^{-1}$ , see text). Note the different vertical scales $^\textrm{\scriptsize 2}$ .
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$\begin{figure} \par\includegraphics[width=8.8cm,clip]{odin6_f6.eps} \end{figure}$	Figure 6: The spectra of Fig. 4 scaled $^\textrm{\scriptsize 2}$ according to the legend. Note that the SiO profile was corrected for the OSO 20 m beam efficiency before scaling.
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